Limit on the brightness of the optical counterpart of the new LMXB in the globular cluster NGC 6440

Details Limit on the brightness of the optical counterpart of the new LMXB in the globular cluster NGC 6440 Limit on the brightness of the optical counterpart of the new LMXB in the globular cluster NGC 6440

Aug 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009atel.2144....1l&link_type=abstract

The Astronomer's Telegram, #2144

Astronomy and Astrophysics

Astronomy

1

Optical, Globular Clusters, Neutron Stars, Transients, Variables

Scientific paper

We report on optical observations of the new LMXB in the globular cluster NGC 6440 announced by Heinke & Budac (2009, Atel 2139) and Heinke et al. (2009, Atel 2143). Observations were performed with the 0.76-m Katzman Automatic Imaging Telescope (KAIT) at Lick Observatory on Jul 30 and 31 UT in the unfiltered mode. A series of 30 s exposures was obtained and stacked, yielding a total exposure of 180 s on Jul 30 and 300 s on Jul 31.

Affiliated with

Also associated with

No associations

Rating

Limit on the brightness of the optical counterpart of the new LMXB in the globular cluster NGC 6440 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Limit on the brightness of the optical counterpart of the new LMXB in the globular cluster NGC 6440, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Limit on the brightness of the optical counterpart of the new LMXB in the globular cluster NGC 6440 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-818905